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TESS Hunt for Young and Maturing Exoplanets (THYME). IX. A 27 Myr Extended Population of Lower Centaurus Crux with a Transiting Two-planet System

Authors: Mackenna L. Wood, Andrew W. Mann, Madyson G. Barber, Jonathan L. Bush, Adam L. Kraus, Benjamin M. Tofflemire, Andrew Vanderburg, Elisabeth R. Newton, Gregory A. Feiden, George Zhou, Luke G. Bouma, Samuel N. Quinn, David J. Armstrong, Ares Osborn, Vardan Adibekyan, Elisa Delgado Mena, Sergio G. Sousa, Jonathan Gagné, Matthew J. Fields, Reilly P. Milburn, Pa Chia Thao, Stephen P. Schmidt, Crystal L. Gnilka, Steve B. Howell, Nicholas M. Law, Carl Ziegler, César Briceño, George R. Ricker, Roland Vanderspek, David W. Latham, Sara Seager, Joshua N. Winn, Jon M. Jenkins, Joshua E. Schlieder, Hugh P. Osborn, Joseph D. Twicken, David R. Ciardi, Chelsea X. Huang

Mackenna L. Wood et al 2023 The Astronomical Journal 165 .

Provider: AAS Journals

Caption: Figure 1.

The results of Comove. HD 109833 and neighbors within 30 pc and 2 km s⁻¹, are shown in X-, Y-, and Z-coordinates. The size of the points corresponds inversely to their distance from HD 109833, and the color with the velocity difference, so that the largest points are closest to HD 109833, and the darkest points are most similar in velocity. Stars with Gaia renormalized unit weight error (RUWE) ≥ 1.2 are represented with squares. The velocity differences of binary stars are poor indicators of membership, due to velocity from binary motion. Circles are used to represent stars with Gaia RUWE < 1.2.

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